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20162026
most citedGravitational waves from supermassive stars collapsing to a supermassive black hole

71 citations · 175 across the 7 of their papers we have counts for

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Showing astro-ph.HEShow all

5 papers · 1 filter

astro-ph.HE2019★ 1 cited

Gravitational waves from very massive stars collapsing to a black hole

Haruki Uchida, Masaru Shibata, Koh Takahashi +1

We compute gravitational waves emitted by the collapse of a rotating very massive star (VMS) core leading directly to a black hole in axisymmetric numerical-relativity simulations.…

astro-ph.HE2018★ 12 cited

Black Hole Formation and Explosion from Rapidly Rotating Very Massive Stars

Haruki Uchida, Masaru Shibata, Koh Takahashi +1

We explore the formation process of a black hole (BH) through the pair-instability collapse of a rotating Population III very massive star in axisymmetric numerical relativity. As…

astro-ph.HE2017★ 51 cited

Gravitational Collapse of Rotating Supermassive Stars including Nuclear Burning Effects

Haruki Uchida, Masaru Shibata, Takashi Yoshida +2

Supermassive stars (SMSs) of mass are candidates for seeds of supermassive black holes found in the center of many massive galaxies. We simulate the gravitat…

astro-ph.HE2016★ 71 cited

Gravitational waves from supermassive stars collapsing to a supermassive black hole

Masaru Shibata, Yuichiro Sekiguchi, Haruki Uchida +1

We derive the gravitational waveform from the collapse of a rapidly rotating supermassive star (SMS) core leading directly to a seed of a supermassive black hole (SMBH) in axisymme…

astro-ph.HE2016★ 23 cited

Stability of rigidly rotating supermassive stars against gravitational collapse

Masaru Shibata, Haruki Uchida, Yuichiro Sekiguchi

We revisit secular stability against quasi-radial collapse for rigidly rotating supermassive stars (SMSs) in general relativity. We suppose that the SMSs are in a nuclear-burning p…